Localized packets of electrostatic whistler emissions near the lower h
ybrid frequency have been observed in the low-attitude auroral region
by sounding rockets and the Freja satellite. We present a model for wa
ve localization that requires two ion species, O+ and H+, whereby the
minority H+ ions control the localization process. The theoretical bas
is is that the plasma dispersion is dramatically affected by small cha
nges in the H+ density and that the observed emissions would selective
ly heat H+. We show observational support for the proposed model.